Energy of Kerr-Newman Black-Holes and Gravitomagnetism
| dc.creator | Berman, Marcelo Samuel | |
| dc.date | 2004-07-07 | |
| dc.date | 2004-08-11 | |
| dc.date.accessioned | 2026-07-07T03:28:50Z | |
| dc.date.available | 2026-07-07T03:28:50Z | |
| dc.description | New formulae are obtained for the energy of K.N. b.h.'s that point out a gravitomagnetic energy effect. The results are valid for slowly or rapidly rotating black-holes. The expression of the energy density of Kerr-Newman back-holes in the slow rotation case, is obtained afterwards, and shown to be essentially positive. Subsequently,we show how to attain a "repulsive" gravitation (antigravitation) state identified with negative energy distribution contents in a limited region of space, without violating the Positive Energy Theorem. | |
| dc.description | 6 pages including front cover | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0407026 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0407026 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/34985 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Energy of Kerr-Newman Black-Holes and Gravitomagnetism | |
| dc.type | text |